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Statistical properties of photons in a three-level plus two-mode model

N.N. Bogolubov, Fam Le Kien, A.S. Shumovsky

To cite this version:

N.N. Bogolubov, Fam Le Kien, A.S. Shumovsky. Statistical properties of photons in a three-level plus two-mode model. Journal de Physique, 1986, 47 (3), pp.427-435. �10.1051/jphys:01986004703042700�.

�jpa-00210222�

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Statistical properties of photons in a three-level plus two-mode model

N. N. Bogolubov Jr., Fam Le Kien and A. S. Shumovsky

Laboratory of Theoretical Physics, Joint Institute for Nuclear Research,

P.O. Box 79, 101 000, Moscow, U.S.S.R.

(Reçu le 22 juillet 1985, révisé le 12 novembre, accepté le 19 novembre 1985)

Resume.

2014

On étudie les caractéristiques des propriétés statistiques des photons dans un modèle analytique à

trois niveaux et deux modes du champ. Le modèle consiste en un émetteur unique, à trois niveaux en lambda, initialement dans le niveau le moins excité, interagissant avec deux modes du champ quantifié. On calcule les variances, en ordre normal, du nombre de photons et les fonctions de corrélation croisées. Tous les résultats sont obtenus sans utiliser, ni théorie de perturbation, ni d’approximations de décorrélation. On montre que les états du mode « signal » du champ, obtenus à partir du vide initial, sont sub-poissoniens à tout instant On décrit l’évo- lution des propriétés statistiques des photons quand le mode « signal » et le mode « pompe » sont initialement dans un état cohérent de Glauber. Dans des conditions convenables, on pourrait obtenir dans ce système, un dégroupement de photons et une anti-corrélation entre les modes.

Abstract

2014

The characteristics of the photon statistical properties are studied in a soluble three-level plus two-

mode model. The model consists of a single lambda-configuration three-level emitter interacting with two modes

of the quantized radiation field, the emitter being initially in the lowest level. The normally ordered variances of the photon numbers and the cross-correlation function are calculated All the results are obtained without using perturbation theory and decorrelation approximations. It is shown that the states of the signal-mode field pro- duced from its initial vacuum are sub-Poissonian for all times. For the case when both the signal-mode and pump- mode fields are initially in the Glauber coherent states the temporal behaviour of the photon statistical characteris- tics are described Under suitable conditions photon antibunching and anticorrelation between the modes are

potentially possible in the system.

Classification

Physics Abstracts

32.80

-

42.50

1. Introduction.

During ten last years the photon antibunching effect

has attracted considerable interest, since it has no

counterpart in classical electrodynamics and, hence, provides new evidence of the wave-particle dualism.

Photon antibunching is characterized by a nonclassi-

cal state of the field in which the variance of the num-

ber of photons is less than the mean number of pho-

tons, i.e. the photons exhibit sub-Poissonian statistics.

While experiments thus far are restricted to the study

of resonance fluorescence from single atoms [1-3],

various physical mechanism that generate such a

state have been shown to be theoretically possible (see Refs. [4-20] and the reviews [21, 22]). Among

them are second harmonic generation [4-7] and three-

wave parametric interaction [8] in a nonlinear medium,

resonance fluorescence from two-level atoms [9-15], degenerate four-wave mixing [16], two-photon absorp-

tion [17, 18], free-electron-laser generation [19, 20].

Recently, the generation of squeezed states, another class of nonclassical states [28], has also become the

object of active researches (see [28-30] and refs.

therein).

In this paper the production of sub-Poissonian non-classical states by using two-mode processes in a three-level system will be discussed. On the basis of the exactly soluble model, studied in [23] we shall

examine the time behaviour of the normally ordered

variances of the photon numbers and of the cross correlation between the modes. It will be shown that under suitable conditions photon antibunching and

anticorrelation between the modes are possible in

the system.

The remainder of the paper is organized as follows.

In section 2 the model Hamiltonian and the necessary

previous results are given. In section 3 we study the

time behaviour of the normally ordered variances of the photon numbers. In section 4 the cross correlation between the modes is calculated Finally, the conclu- sions are briefly summarized in section 5.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01986004703042700

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428

2. Model Hamiltonian and basic equations.

-

The lambda-configuration three-level emitter considered here is shown in figure 1. The upper level 3 is connected with the levels 1 and 2 by dipole transitions whereas the transition 1-2 is forbidden. The Hamiltonian

describing the interaction of the emitter with the two-mode resonant radiation field in the dipole and rotating wave approximations is [23]

Here, the operator Rjj = I j) j I describes the

population of level j with the corresponding energy

1iQj and state vector I j). Rij * [ i ) j I is the ope- rator of transition from level j to level i. The operators

Rij, i, j = 1, 2, 3, obey the following relations :

The photon operators âa, â: describe two modes of

the radiation field with the resonance frequencies (J)a = D3 - Da, and ga’s are the corresponding para- meters of emitter-mode coupling.

The three-level two-mode model (1) has extensively

been investigated [31, 23] (see also [32] and Refs.

therein). In the framework of this model one can

study not only various purely quantum effects in

population dynamics and photon statistics [31, 34]

but also fine features in indirect two-mode interaction

Fig. 1.

-

Energy level structure of the lambda configuration

emitter interacting with the two-mode resonant radiation

field.

via the emitter. An excellent review of the dynamical theory of the model has recently been given by Yoo

and Eberly in paper [31]. Nonclassical photon sta-

tistics has been numerically shown. However, these authors do not make any comments about it. Some discussions about experimental verifications, being possible due to progress in the realization of a single

atom in a cavity [33-37], have been given in refe-

rence [31]. We shall study the time behaviour of

photon statistics and mode correlations below.

We assume that the emitter is initially on the

lowest level 1. In the papers [23] the time-dependent

two-mode photon-distribution function Plnl’ n2) has

been found explicitly and rigorously. It reads

where

and the function P(ni, n2) = Pt=O(nl’ n2) is the initial photon distribution. In general case, for an arbitrary

initial field state described by a density matrix PF we have

Starting from equations (3. 5), we shall examine photon statistics of the modes in the remainder of this

paper.

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3. Normally ordered variances of the numbers of the photons in the modes.

From equation (3) one easily finds the normally ordered variance Vjsj of the photon number in the signal mode (mode 2)

The expression of the corresponding quantity V,Pl for the pump mode (mode 1) is found from equation (3) to be

Here,

and

denote the mean numbers of the initial photons in

the pump and signal modes, respectively.

As is well known, the quantities Vjsj and V [P)

characterize the photon statistical properties of the

modes. They are proportional to the excess coinci-

dence counting rates to be measured in a Hanbury

Brown and Twiss-type [24, 25] experiment. The sign plus or minus or Vjsj (or V[P]) shows the photon sta-

tistics of the signal (or pump) mode is super- or sub- Poissonian and indicates, therefore, whether bunching (+) or antibunching (-) occurs [21, 22]. Now, we consider some consequences of the expressions (6)

and (7).

First of all note that if the signal mode 2 is initially

in the vacuum state, i.e. P(nl, n2)

=

bn2o P(ni), from

(6) we have

This implies that the signal light field generated from

the initial vacuum by arbitrary light pumping has

sub-Poissonian photon statistics and, hence, exhibits photon antibunching for all times t > 0. In figure 2

we plot V[S] versus time go t for the case of coherent

pumping with

Fig. 2.

-

Temporal behaviour of the normally ordered

variance V[S](t) of the photon number in the signal-mode

fied produced from the vacuum by Glauber-coherent

pumping. Calculations are performed for g1

=

g2 = go,

P(n1’ n2) = ðn20 P(n1) P(n1) = exp(- ’l) fill’ll and n1

=

12. Time is measured in units of 1/go.

and n-1

=

12. The figure shows distinctly the Rabi

non linear oscillations, collapse and revival of their

envelopes (see [26] and below).

Let us now assume that both the signal and pump modes are initially in Glauber states I z, > and z2 >, respectively. This means, the initial distribution

P(ni, n2) of the photon numbers in the modes is given

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430

by

Substituting (9) into (6) and (7), we perform a nume-

rical examination for visi and vipi In figure 3 we

plot these quantities as functions of time for g2 =

29t = 2 go, n2 = 9, ii, = 4. For very short times

(0 go t 0.25), the value of V[s] is positive, whilst

the value of V [P] is negative. As time goes on (go t 3),

we observe oscillations of both the values and their

corresponding signs (see Fig. 3a). From the figure it is

clear that sub-Poissonian photon statistics and anti-

bunching in the modes occur for some finite inter- vals. Such a time behaviour of photon statistics is connected with the so-called Rabi oscillations [21, 22, 26]. For longer times (go t > 3) Vjsj and V [P]

reach the steady values. This corresponds to the Cummings collapse region 26. The negative steady

value Vo predicts antibunching in the signal mode.

The stationary behaviour of the variances continues until the appearance of revivals [26], see figure 3b,

where they start oscillating again. Thus, we see that

in the considered case, when g2 n2/gî ni = 9 » 1 antibunching in the signal mode takes place both

in the Rabi oscillation region and during the collapse

and revival. An analytic approximate description of

the above-obtained numerical results can be given

in the following.

Due to the well-known properties of the two-

dimension Poissonian distribution (9)

from equations (6) and (7) we have

Here, for convenience the notation (...) == L P(nl, n2) (...) has been introduced

Ill,n2

In the case nl’ n2 > 1 the summations over n, and n2 in (11) can be performed approximately by using saddle-point techniques [26] if one notices that the weighting factor P(ni, n2) will peak at (n1, n2) with relatively

narrow dispersion. This means that the expressions in (11) can be changed to integrals of fast oscillating functions

which after trivial transformations can be written as

with (see [26])

Note that the function F(t; g2) approaches unity in the limit t -+ oo. Then we can easily find from equations (12)

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analytical approximate expressions for the steady values V0[s] and VI of the variances. They read

V,, -

.

Fig. 3.

-

Time dependence of the normally ordered va-

riances V.(i) and Vlp,(t) of the photon numbers in the signal

and pump modes, respectively. Both the fields of the modes

are initially in the Glauber coherent states with nl

=

4,

n2

=

9, gt

=

0.5 g2 z go. Time is measured in units of

1/go. (a) Short times : go t 5. In this case the basic oscillations occur at the Rabi frequencies, and are subject

to Gaussian collapse resulting in the steady behaviour.

(b) Long times : the range of time is eight times larger than in (a). The long time behaviour is characterized by revival.

We plot the quantity Vo as a function of n2 in figure 4a

(for ni = 10, gt = 92 = go) and as a function of

n1 in figure 4b (for n2 = 0,10, gi = g2 = go). From

Fig. 4.

-

Steady value V&J of the normally ordered variance of the photon number in the signal mode. (a) The depen-

dence of V&J upon n2 in the case 91

=

g2, n1

=

10. (b) The dependence of Vo upon nl in the cases when g1 = 92’

n2 = 0 and 10.

the figures we see that Vo is negative for very small

values n2 (n2 = 0) and for large values n2 as compar- ed with ii, 2 n2 g21 n1). By using the first equa- tion in (15) we can easily get the estimate

for the case g2 - >> g2 -1. On the other hand, for

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432

the case when the initial state of the signal mode field

is vacuum or near-vacuum, Le. n2 0, and when n, > 1, we find straight forwardly from equation (11)

the evaluation

(which is also in compliance with the first equation

in (15) in the limit n-2 --+ 0). The inequalities in equa- tions (16) and (17) mean that photon statistics of the

signal mode field in the steady regime will be sub- Poissonian if either g’ 2 n- 2 >> 9 2 1 n, (n-,, n- 2 1) or n2 - 0, Ei » 1. This confirms the numerical results obtained above, see figures 2, 3 and 4.

For short times and large initial photon numbers ni, n2 by using the saddle-point method for evaluating

the integral (13), one can get

The right-hand side of equation (18) behaves like

damped cosine oscillations which are terminated

by the Gaussian envelope exp[ - t2/(2 t2c)]. Here

the collapse time Tc is defined as

The approximate expression (18) together with equa- tions (12) give a description of the behaviour of the variances V[s], V [P] in the short time regime t l’ c

(see Fig. 3a). In particular, for early time t = 0 we

can obtain

Emphasize that the approximate expression (18)

is not valid in the long time region. Therefore, it

cannot describe the revival of the oscillation envelopes

of VIS] and V[P], which occurs when t >> LC’ see figure 3b.

Applying the long-time approximate method deve-

loped on the basis of the saddle-point method by Eberly and his coworkers in reference [26] to calcu-

late the integral (13) we can get in the special case 91 = 92 =- go the following evaluation

where the notation

has been introduced, and

The approximate expression (21) is rather good for all times [26]. It indicates the periodicity of the revivals. The interval TR between the revivals of the oscillation envelope of F(t; g2) can be found from the second equation

in (22) to be

4. Cross correlation.

More interesting is the cross correlation between the two modes. Its magnitude can be characterized by

The quantity Vcross is proportional to the excess coincidence counting rate to be measured in an experiment

of the Hanbury Brown-Twiss-type with two different light beams [22, 27]. We speak of anticorrelation, when Vcross becomes negative. Anticorrelation has been observed in light scattering from nonspherical particles in

dilute solution [27]. We consider now the time behaviour of Vcross in the model (1).

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Utilizing equation (3) and the definition (25) we can get

Equation (26) together with equations (4) allow us to describe the time evolution of the cross correlation in the

general case of the initial field state (5). Let us assume that the initial photon distribution P(n1, n2) is given by (9).

This means that the signal and pump fields are coherent and statistically independent at the beginning of the

interaction. Then, due to the properties (10), we find from (26) the result

Here (...) indicates, as in section 3, averaging over the distribution (9).

A numerical computation of the formula (27) has been performed for the case, for example, when g1

=

2g2 =

2 go, ni = 12, n2 = 3. The results are plotted in figure 5. We see from the figure that anticorrelation occurs for

some finite intervals of times in the Rabi oscillation region, and during the steady regime. The successive pre-

sences of correlation and anticorrelation in the Rabi oscillation region are noted For large photon numbers ni, n2 by using the approximate formulae

obtained from (4), we can apply the same analytical description we have used in the previous section to (27).

The collapse and revival of Vcross are easily described by utilizing the approximate expressions (18) and (21).

Due to that the function F(t; g2) approaches unity in the collapse region, see (18), and in the region of infinitely large times, see (21), the steady value of V cross is quickly found to be

Fig. 5.

-

Time evolution of the cross-correlation function

Vcross(t). Both the fields of the modes are initially in the

Glauber coherent states with nl

=

12, n2

=

3, gl

=

2 g2 =

2 go. Time is measured in units of 1/g0.

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434

Hence, for the case g’ 1 ;il >> g2 n2 one gets

The inequality in equation (30) indicates the anti- correlation between the signal and pump modes in the steady regime. This analytical prediction is in compliance with the numerical result obtained above,

see figure 5 (where gf nl/gi n2 = 16). In the opposite

limit case g2 jil g2 n2 one has

that indicates the correlation between the modes.

Finally, for very short times t 0 we find from

equations (27) and (4) the formula

which describes the appearance of the correlation between the modes due to the interaction with the

emitter, see figure 5.

5. Conclusions.

In this paper we have studied the characteristics of the photon statistical properties in a soluble three-

level plus two-mode model. The normally ordered

variances of the photon numbers and the cross- correlation function have been calculated It has been

shown that the states of the signal mode field pro- duced from its initial vacuum are sub-Poissonian for all times. This production of sub-Poissonian states

does not depend upon the initial state of the pump mode field

The quantum collapse and revival behaviour of the

photon statistical characteristics in the lossless model considered here have been noted

For the case when both the signal-mode and pump- mode fields are initially in the Glauber coherent

states the time behaviour of the photon-number

variances and of the cross correlation between the modes has been numerically examined and analyti- cally approximated The theoretical investigations

show that under suitable conditions the occurrence

of photon antibunching and the presence of anti- correlation between the modes are potentially possible

in the system. It has been established that

(i) In the region of short times (the Rabi oscilla-

tion region) photon statistics of the signal-mode

field is sub-Poissonian for some finite intervals;

(ii) Photon statistics of the signal-mode field in the

steady regime will de sub-Poissonian if either g’ - 91 2 ;il (n-1, ;i2 > 1) or ;i2 = 0 (n-, >> 1);

(iii) Due to the interaction with the emitter the correlations between the modes come into existence.

The anticorrelation between the modes will occur in the steady regime if g 1 n 1 > g2 n2 (n-" - n2 >> 1 ).

All the results have been obtained without using perturbation theory and decorrelation approxima-

tions.

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